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Title: AN EXTREME GRAVITATIONALLY REDSHIFTED IRON LINE AT 4.8 KeV IN Mrk 876

Abstract

X-ray spectral lines at unforeseen energies are important because they can shed light on the extreme physical conditions of the environment around the supermassive black holes of active galactic nuclei (AGNs). Mrk 876 displays such a line at 4.80{sub −0.04}{sup +0.05} rest-frame energy. A possible interpretation of its origin can be found in the hotspot scenario. In this scenario, the primary radiation from a flare in the hot corona of an AGN illuminates a limited portion of the accretion disk that emits by fluorescence. In this context, the line can represent an extreme gravitationally redshifted Fe line originating on the accretion disk below six gravitational radii from a rotating supermassive black hole. The correct estimate of the line significance requires a dedicated approach. Based on an existing rigorous approach, we have performed extensive Monte Carlo simulations. We determine that the line is a real feature at a ∼99% confidence level.

Authors:
; ;  [1];  [2];  [3];  [4]
  1. W. W. Hansen Experimental Physics Laboratory and Kavli Institute for Particle Astrophysics and Cosmology, Stanford University (United States)
  2. Max-Planck-Institut für extraterrestrische Physik, Giessenbachstrasse 1, D-85748 Garching (Germany)
  3. Department of Physics and Astronomy, Clemson University, Clemson, SC 29634-0978 (United States)
  4. INAF-Trieste, via G.B.Tiepolo 11, I-34143 Trieste (Italy)
Publication Date:
OSTI Identifier:
22364738
Resource Type:
Journal Article
Resource Relation:
Journal Name: Astrophysical Journal Letters; Journal Volume: 798; Journal Issue: 1; Other Information: Country of input: International Atomic Energy Agency (IAEA)
Country of Publication:
United States
Language:
English
Subject:
79 ASTROPHYSICS, COSMOLOGY AND ASTRONOMY; ACCRETION DISKS; BLACK HOLES; COMPUTERIZED SIMULATION; FLUORESCENCE; GALAXY NUCLEI; IRON; KEV RANGE; MONTE CARLO METHOD; ORIGIN; RED SHIFT; STELLAR FLARES; VISIBLE RADIATION; X-RAY GALAXIES; X-RAY SPECTRA

Citation Formats

Bottacini, Eugenio, Orlando, Elena, Moskalenko, Igor, Greiner, Jochen, Ajello, Marco, and Persic, Massimo, E-mail: eugenio.bottacini@stanford.edu. AN EXTREME GRAVITATIONALLY REDSHIFTED IRON LINE AT 4.8 KeV IN Mrk 876. United States: N. p., 2015. Web. doi:10.1088/2041-8205/798/1/L14.
Bottacini, Eugenio, Orlando, Elena, Moskalenko, Igor, Greiner, Jochen, Ajello, Marco, & Persic, Massimo, E-mail: eugenio.bottacini@stanford.edu. AN EXTREME GRAVITATIONALLY REDSHIFTED IRON LINE AT 4.8 KeV IN Mrk 876. United States. doi:10.1088/2041-8205/798/1/L14.
Bottacini, Eugenio, Orlando, Elena, Moskalenko, Igor, Greiner, Jochen, Ajello, Marco, and Persic, Massimo, E-mail: eugenio.bottacini@stanford.edu. Thu . "AN EXTREME GRAVITATIONALLY REDSHIFTED IRON LINE AT 4.8 KeV IN Mrk 876". United States. doi:10.1088/2041-8205/798/1/L14.
@article{osti_22364738,
title = {AN EXTREME GRAVITATIONALLY REDSHIFTED IRON LINE AT 4.8 KeV IN Mrk 876},
author = {Bottacini, Eugenio and Orlando, Elena and Moskalenko, Igor and Greiner, Jochen and Ajello, Marco and Persic, Massimo, E-mail: eugenio.bottacini@stanford.edu},
abstractNote = {X-ray spectral lines at unforeseen energies are important because they can shed light on the extreme physical conditions of the environment around the supermassive black holes of active galactic nuclei (AGNs). Mrk 876 displays such a line at 4.80{sub −0.04}{sup +0.05} rest-frame energy. A possible interpretation of its origin can be found in the hotspot scenario. In this scenario, the primary radiation from a flare in the hot corona of an AGN illuminates a limited portion of the accretion disk that emits by fluorescence. In this context, the line can represent an extreme gravitationally redshifted Fe line originating on the accretion disk below six gravitational radii from a rotating supermassive black hole. The correct estimate of the line significance requires a dedicated approach. Based on an existing rigorous approach, we have performed extensive Monte Carlo simulations. We determine that the line is a real feature at a ∼99% confidence level.},
doi = {10.1088/2041-8205/798/1/L14},
journal = {Astrophysical Journal Letters},
number = 1,
volume = 798,
place = {United States},
year = {Thu Jan 01 00:00:00 EST 2015},
month = {Thu Jan 01 00:00:00 EST 2015}
}